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CETP, IPSL, Saint Maur, France
IPSL / CETP, 4, avenue de Neptune, Saint-Maur des Fosse, F-94107 France / IPSL-CNRS, 4, Avenue de Neptune, 94107 Saint Maur, France
CETP-IPSL, 4, avenue de Neptune, Orléans, 94107 France; LPCE-CNRS, 3A, avenue de la Recherche, Orléans, 45100 France 4, Avenue de Neptune, Saint Maur, 94107, France 4 Avenue de Neptune, 94107, Saint-Maur Cedex, France
LATMOS-IPSL, Saint-Maur des Fosses cedex, France
LATMOS / IPSL, CNRS-UVSQ-UPMC, 4 avenue de Neptune, 94107 Saint-Maur, France
Centre d'Étude des Environnements Terrestre et Planetaires, 4 avenue de Neptune, Saint Maur, 94107, France 4, Avenue de Neptune, Saint Maur, 94107, France d'Études des Environnements Terrestres et Planétaires, Centre National de la Recherche Scientifique, Institut Pierre-Simon Laplace, France, 4 avenue de Neptune, F-94107 Saint-Maur-des-Fossés, France
CETP, IPSL, CNRS, Saint Maur, France
CNRS, Laboratoire de Physique et de Chimie de l'Environnement, Orleans, France
Centre de Recherches en Physique de l'Environnement, Issy-les-Moulineaux, France
Centre d'Études des Environnements Terrestre et Planétaires
CNRS, LATMOS, Paris, France
LATMOS / IPSL, Saint Maur, France
Space Science Department, ESA / ESTEC, P.O. Box 299, 2200 AG Noordwijk The Netherlands
Laboratoire de Physique et Chimie de l'Environnement, Orleans, France
Pôle de Planétologie de l'IPSL, Université Pierre et Marie Curie, Boite 102, Service d'Areonomie, 4 place Jussieu, 75252 Paris cedex 05, France
LATMOS-IPSL-Université de Versailles St Quentin, Saint-Maur, France
LATMOS-IPSL, Université Pierre et Marie Curie, 4, Place Jussieu, 75252 Paris Cedex 05, France
CETP, France
Université Vesailles St. Quentin, CNRS / INSU, LATMOS-IPSL, France
A comparison between the earth's and Mars' bow shocks detected by the PHOBOS Plasma-Wave System
A ground penetrating radar to explore the Martian subsurface.
A new approach for estimating Titan's electron conductivity based on data from relaxation probe sensors on the Huygens experiment
A new numerical model for the simulation of ELF wave propagation and the computation of eigenmodes in the atmosphere of Titan: Did Huygens observe any Schumann resonance?
A Schumann-like resonance on Titan driven by Saturn's magnetosphere possibly revealed by the Huygens Probe
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